Icy bodies, such as Pluto, are known to harbor simple and complex molecules. The recent New Horizons flyby of Pluto has revealed a complex surface composed of bright and dark ice surfaces, indicating a rich chemistry based on nitrogen (N2), methane (CH4), and carbon monoxide (CO). Nitrile (CN) containing molecules such as acetonitrile (CH3CN), propionitrile (CH3CH2CN), butyronitrile (CH3CH2CH2CN), and isobutyronitrile ((CH3)2CHCN) are some of the nitrile molecules that are known to be synthesized by radiative processing of such simple ices. Through the provision of a spectral atlas for such compounds we propose that such nitriles may be identified from the ALICE payload on board New Horizons
The chemical composition of protoplanetary disks around young stars affects the chemical habitabilit...
Context: One of the main scientific objectives of NASA's New Horizons mission is to map the icy surf...
Aims. Spectroscopic investigation of the surface of Pluto allows us to constrain the chemical proper...
Icy bodies, such as Pluto, are known to harbor simple and complex molecules. The recent New Horizons...
Here we present the first Vacuum UltraViolet (VUV) photoabsorption spectra of ice analogues of Pluto...
The information we have on the chemical compositions of the surfaces of Pluto and Charon has been ob...
Radiation processing of the surface ices of outer solar system bodies may result in the production o...
Pluto's bulk composition and the composition of the surface layers hold clues to the origin and evol...
94035We report on our analysis of blended Pluto and Charon spectra over the wavelength range 1.4 to ...
The recent discovery of two large trans-Neptunian objects (TNOs) 2003 UB313 and 2005 FY9, with surfa...
Much of the surface of Pluto consists of high-albedo regions covered to an unknown depth by Beta-N2,...
© 2016 From Earth based observations Pluto is known to be the host of N2, CH4 and CO ices and also a...
We have obtained spectra of the Pluto-Charon pair (unresolved) in the wavelength range 380-930 nm wi...
Pluto is a large icy body composed of N$_{2}$, CH$_{4}$, and H$_{2}$O ices. In many ways, Pluto can ...
Tholins are refractory organic solids of complex structure and high molecular weight, with a wide ra...
The chemical composition of protoplanetary disks around young stars affects the chemical habitabilit...
Context: One of the main scientific objectives of NASA's New Horizons mission is to map the icy surf...
Aims. Spectroscopic investigation of the surface of Pluto allows us to constrain the chemical proper...
Icy bodies, such as Pluto, are known to harbor simple and complex molecules. The recent New Horizons...
Here we present the first Vacuum UltraViolet (VUV) photoabsorption spectra of ice analogues of Pluto...
The information we have on the chemical compositions of the surfaces of Pluto and Charon has been ob...
Radiation processing of the surface ices of outer solar system bodies may result in the production o...
Pluto's bulk composition and the composition of the surface layers hold clues to the origin and evol...
94035We report on our analysis of blended Pluto and Charon spectra over the wavelength range 1.4 to ...
The recent discovery of two large trans-Neptunian objects (TNOs) 2003 UB313 and 2005 FY9, with surfa...
Much of the surface of Pluto consists of high-albedo regions covered to an unknown depth by Beta-N2,...
© 2016 From Earth based observations Pluto is known to be the host of N2, CH4 and CO ices and also a...
We have obtained spectra of the Pluto-Charon pair (unresolved) in the wavelength range 380-930 nm wi...
Pluto is a large icy body composed of N$_{2}$, CH$_{4}$, and H$_{2}$O ices. In many ways, Pluto can ...
Tholins are refractory organic solids of complex structure and high molecular weight, with a wide ra...
The chemical composition of protoplanetary disks around young stars affects the chemical habitabilit...
Context: One of the main scientific objectives of NASA's New Horizons mission is to map the icy surf...
Aims. Spectroscopic investigation of the surface of Pluto allows us to constrain the chemical proper...